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Ballooning instability in the presence of a plasma flow: A synthesis of tail reconnection and current disruption models for the initiation of substorms

MPS-Authors
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Korth,  A.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Zong,  Q.-G.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Friedel,  R. H. W.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Pu, Z. Y., Kang, K. B., Korth, A., Fu, S. Y., Zong, Q.-G., Chen, Z. X., et al. (1999). Ballooning instability in the presence of a plasma flow: A synthesis of tail reconnection and current disruption models for the initiation of substorms. Journal Geophysical Research, 104(A5), 10235-10248.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-DB5B-6
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